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Excitation of a Primordial Cold Asteroid Belt as an Outcome of Planetary Instability

Astrophysical journal. Letters, 2018-09, Vol.864 (1), p.50

2018

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Constraining the Giant Planets' Initial Configuration from Their Evolution: Implications for the Timing of the Planetary Instability

The Astronomical journal, 2017-04, Vol.153 (4), p.153-153

2017

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The observation of large semi-major axis Centaurs: Testing for the signature of a planetary-mass solar companion

Icarus (New York, N.Y. 1962), 2015-09, Vol.258, p.37-49

2015

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Is the Grand Tack model compatible with the orbital distribution of main belt asteroids?

Icarus (New York, N.Y. 1962), 2016-07, Vol.272, p.114-124

2016

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Evidence from the Asteroid Belt for a Violent Past Evolution of Jupiter's Orbit

The Astronomical journal, 2010-11, Vol.140 (5), p.1391-1401

2010

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The origin of the Kuiper Belt high–inclination population

Icarus (New York, N.Y. 1962), 2003-02, Vol.161 (2), p.404-418

Gomes, Rodney S

2003

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The origin of TNO 2004 XR190 as a primordial scattered object

Icarus (New York, N.Y. 1962), 2011-10, Vol.215 (2), p.661-668

GOMES, Rodney S

2011

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The formation of the cold classical Kuiper Belt by a short range transport mechanism

Icarus (New York, N.Y. 1962), 2021-03, Vol.357, p.114121, Article 114121

Gomes, Rodney

2021

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Planetary migration in a planetesimal disk: why did Neptune stop at 30 AU?

Icarus (New York, N.Y. 1962), 2004-08, Vol.170 (2), p.492-507

2004

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Was Triton originally a regular satellite of Neptune?

Icarus (New York, N.Y. 1962), 2024-09, Vol.420, p.116142, Article 116142

2024

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The evolution of a Pluto-like system during the migration of the ice giants

Icarus (New York, N.Y. 1962), 2015-01, Vol.246, p.330-338

2015

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THE INCLINATION OF THE PLANETARY SYSTEM RELATIVE TO THE SOLAR EQUATOR MAY BE EXPLAINED BY THE PRESENCE OF PLANET 9

The Astronomical journal, 2017-01, Vol.153 (1), p.27-27

2017

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A distant planetary-mass solar companion may have produced distant detached objects

Icarus (New York, N.Y. 1962), 2006-10, Vol.184 (2), p.589-601

2006

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On The Origin of The High-Perihelion Scattered Disk: The Role of The Kozai Mechanism And Mean Motion Resonances

Celestial mechanics and dynamical astronomy, 2005-01, Vol.91 (1-2), p.109-129

2005

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Dynamical evidence for an early giant planet instability

Icarus (New York, N.Y. 1962), 2020-03, Vol.339, p.113605, Article 113605

2020

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The Influence of Planet Nine on the Orbits of Distant TNOs: The Case for a Low-perihelion Planet

The Astronomical journal, 2018-10, Vol.156 (4), p.157

2018

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On the origin of the Kuiper belt

Celestial mechanics and dynamical astronomy, 2009-06, Vol.104 (1-2), p.39-51

Gomes, Rodney da Silva

2009

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Checking the compatibility of the cold Kuiper belt with a planetary instability migration model

Icarus (New York, N.Y. 1962), 2018-05, Vol.306, p.319-327

2018

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Late Orbital Instabilities in the Outer Planets Induced by Interaction with a Self-gravitating Planetesimal Disk

The Astronomical journal, 2011-11, Vol.142 (5), p.152-jQuery1323896812661='48'

2011

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Origin of the structure of the Kuiper belt during a dynamical instability in the orbits of Uranus and Neptune

Icarus (New York, N.Y. 1962), 2008-07, Vol.196 (1), p.258-273

2008

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Dynamics of the Giant Planets of the Solar System in the Gaseous Protoplanetary Disk and Their Relationship to the Current Orbital Architecture

The Astronomical journal, 2007-11, Vol.134 (5), p.1790-1798

2007

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Constructing the secular architecture of the solar system II: the terrestrial planets

Astronomy and astrophysics (Berlin), 2009-11, Vol.507 (2), p.1053-1065

2009

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Dynamical origin of the Dwarf Planet Ceres

Icarus (New York, N.Y. 1962), 2022-06, Vol.379, p.114933, Article 114933

2022

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Dynamical effects on the classical Kuiper belt during the excited-Neptune model

Icarus (New York, N.Y. 1962), 2019-12, Vol.334, p.89-98

2019

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Constructing the secular architecture of the solar system I. The giant planets

Astronomy and astrophysics (Berlin), 2009-11, Vol.507 (2), p.1041-1052

2009

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Excitation of a Primordial Cold Asteroid Belt as an Outcome of Planetary Instability

Constraining the Giant Planets' Initial Configuration from Their Evolution: Implications for the Timing of the Planetary Instability

The observation of large semi-major axis Centaurs: Testing for the signature of a planetary-mass solar companion

Is the Grand Tack model compatible with the orbital distribution of main belt asteroids?

Evidence from the Asteroid Belt for a Violent Past Evolution of Jupiter's Orbit

The origin of the Kuiper Belt high–inclination population

The origin of TNO 2004 XR190 as a primordial scattered object

The formation of the cold classical Kuiper Belt by a short range transport mechanism

Planetary migration in a planetesimal disk: why did Neptune stop at 30 AU?

Was Triton originally a regular satellite of Neptune?

The evolution of a Pluto-like system during the migration of the ice giants

THE INCLINATION OF THE PLANETARY SYSTEM RELATIVE TO THE SOLAR EQUATOR MAY BE EXPLAINED BY THE PRESENCE OF PLANET 9

A distant planetary-mass solar companion may have produced distant detached objects

On The Origin of The High-Perihelion Scattered Disk: The Role of The Kozai Mechanism And Mean Motion Resonances

Dynamical evidence for an early giant planet instability

The Influence of Planet Nine on the Orbits of Distant TNOs: The Case for a Low-perihelion Planet

On the origin of the Kuiper belt

Checking the compatibility of the cold Kuiper belt with a planetary instability migration model

Late Orbital Instabilities in the Outer Planets Induced by Interaction with a Self-gravitating Planetesimal Disk

Origin of the structure of the Kuiper belt during a dynamical instability in the orbits of Uranus and Neptune

Dynamics of the Giant Planets of the Solar System in the Gaseous Protoplanetary Disk and Their Relationship to the Current Orbital Architecture

Constructing the secular architecture of the solar system II: the terrestrial planets

Dynamical origin of the Dwarf Planet Ceres

Dynamical effects on the classical Kuiper belt during the excited-Neptune model

Constructing the secular architecture of the solar system I. The giant planets

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